From spacetime foam to holographic foam cosmology

May, 2006
8 pages
Published in:
  • Phys.Lett.B 649 (2007) 243-246
e-Print:

Citations per year

2007201120152019202202468
Abstract: (Elsevier)
Due to quantum fluctuations, spacetime is foamy on small scales. For maximum spatial resolution of the geometry of spacetime, the holographic model of spacetime foam stipulates that the uncertainty or fluctuation of distance l is given, on the average, by (llP2)1/3 where lP is the Planck length. Applied to cosmology, it predicts that the cosmic energy is of critical density and the cosmic entropy is the maximum allowed by the holographic principle. In addition, it requires the existence of unconventional (dark) energy/matter and accelerating cosmic expansion in the present era. We will argue that a holographic foam cosmology of this type has the potential to become a full fledged competitor (with distinct testable consequences) for scalar driven inflation.
Note:
  • This paper is dedicated to Rafael Sorkin to celebrate his contibutio contribution to physics: to appear on the Sorkin60 website
  • 04.60.-m
  • 03.67.Lx
  • 95.75.Kk
  • 98.80.-k
  • Holographic model
  • Spacetime foam
  • Critical energy density
  • Dark energy
  • Dark matter
  • space-time: foam